# The cosmic spectral energy distribution in the EAGLE simulation

**Authors:** Maarten Baes (UGent), Ana Tr\v{c}ka (UGent), Peter Camps (UGent),, Angelos Nersesian (UGent, NOA Athens), James Trayford (Leiden), Tom Theuns, (ICC, Durham), Wouter Dobbels (UGent)

arXiv: 1901.08878 · 2019-02-13

## TL;DR

This study compares the cosmic spectral energy distribution from observations and the EAGLE simulation, finding good agreement at low redshift but discrepancies at higher redshift due to simulation limitations and dust evolution uncertainties.

## Contribution

It demonstrates that combining EAGLE simulation with SKIRT dust modeling produces a realistic local Universe CSED, highlighting areas for improvement at higher redshifts.

## Key findings

- Excellent match with observed CSED at z=0 across UV to submm wavelengths.
- Underestimation of CSED at higher redshift, especially in FIR/submm.
- Discrepancies attributed to simulation volume and dust evolution uncertainties.

## Abstract

The cosmic spectral energy distribution (CSED) is the total emissivity as a function of wavelength of galaxies in a given cosmic volume. We compare the observed CSED from the UV to the submm to that computed from the EAGLE cosmological hydrodynamical simulation, post-processed with stellar population synthesis models and including dust radiative transfer using the SKIRT code. The agreement with the data is better than 0.15 dex over the entire wavelength range at redshift $z=0$, except at UV wavelengths where the EAGLE model overestimates the observed CSED by up to a factor 2. Global properties of the CSED as inferred from CIGALE fits, such as the stellar mass density, mean star formation density, and mean dust-to-stellar-mass ratio, agree to within better than 20 per cent. At higher redshift, EAGLE increasingly underestimates the CSED at optical-NIR wavelengths with the FIR/submm emissivity underestimated by more than a factor of 5 by redshift $z=1$. We believe that these differences are due to a combination of incompleteness of the EAGLE-SKIRT database, the small simulation volume and the consequent lack of luminous galaxies, and our lack of knowledge on the evolution of the characteristics of the interstellar dust in galaxies. The impressive agreement between the simulated and observed CSED at lower $z$ confirms that the combination of EAGLE and SKIRT dust processing yields a fairly realistic representation of the local Universe.

## Full text

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## Figures

5 figures with captions in the complete paper: https://tomesphere.com/paper/1901.08878/full.md

## References

157 references — full list in the complete paper: https://tomesphere.com/paper/1901.08878/full.md

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Source: https://tomesphere.com/paper/1901.08878